Variability of OB stars from TESS southern Sectors 1–13 and high-resolution IACOB and OWN spectroscopy

@article{Burssens2020VariabilityOO,
  title={Variability of OB stars from TESS southern Sectors 1–13 and high-resolution IACOB and OWN spectroscopy},
  author={Siemen Burssens and Sergio Sim'on-D'iaz and Dominic M. Bowman and G. Holgado and Mathias Michielsen and A. de Burgos and Norberto Castro and Rodolfo H. Barb'a and Conny Aerts},
  journal={Astronomy \& Astrophysics},
  year={2020}
}
Context. The lack of high-precision long-term continuous photometric data for large samples of stars has impeded the large-scale exploration of pulsational variability in the OB star regime. As a result, the candidates for in-depth asteroseismic modelling have remained limited to a few dozen dwarfs. The TESS nominal space mission has surveyed the southern sky, including parts of the galactic plane, yielding continuous data across at least 27 d for hundreds of OB stars. Aims. We aim to couple… 

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